Concentration parameter as a tracer of black hole subsystems in globular clusters

Turaev, S.J.

O‘zbekiston fizika jurnali · 2025-yil

Annotatsiya

This study investigates the empirical relationship between the concentration parameter (λ),which characterizes the central stellar density gradient of globular clusters (GCs), and thephysical properties of black hole systems within them. Using structural data derived from surfacedensity profiles observed by HST and Gaia DR2, we computed λ values for 47 GalacticGCs by applying the Nuker model through the simplex optimization method. These λ valueswere then correlated with black hole subsystem (BHS) parameters, such as black hole number,total mass, and relative abundance, obtained from simulation-based studies. These results highlightthe potential of the concentration parameter as a structural diagnostic for inferring thepresence and scale of black hole populations in GCs.

Maqola ma’lumotlari
MualliflarTuraev, S.J.
JurnalO‘zbekiston fizika jurnali
Nashr sanasi2025-10-31
Jild27
Son3
TilIngliz
DOI10.52304/.v27i3.587

Kalit so‘zlar

параметр концентрации, черная дыра звездной массы, система черных дыр, моделирование, concentration parameter, stellar-mass black hole, black hole system, simulation

Ilmiy soha

O‘zbekiston fizika jurnali jurnalidan boshqa maqolalar

O‘zbekiston fizika jurnali — barcha maqolalar